Просмотр архива за воскресенье, 30 октября 2011
Отчет о солнечной активности
Любая солнечная вспышка, упомянутая в этом расчете, имеет масштабирующий коэффициент, применяемый Центром прогнозирования космической погоды (SWPC). Из-за него солнечные вспышки здесь на 42% слабее, чем в научных данных. Из наших архивов этот коэффициент был удален, чтобы показать реальные величины вспышек.
Отчет о солнечно-геофизической активности 2011 Oct 30 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 303 на уровне 2200Z 30 Oct 2011
IA. Анализ активных солнечных регионов и активности от 29 - 2100Z до 30 - 2100Z
Solar activity was low. There were several C-class
flares during the past 24 hours. Most of these were from newly
emerging Region 1334 (N13E24) which is currently a C-type group with
area of about 70 millionths. Region 1330 (N08W35) continues to be
the largest group on the disk and managed to produce two C-class
flares. However, Region 1330 appears to be decreasing in sunspot
area. There continues to be indicators of a new region rotating
around the east limb with latitude around 15 degrees North. A CME
was observed in the LASCO C2 coronagraph beginning at about 0812Z
but was confirmed to be from the backside using STEREO imagery.
IB. Прогноз солнечной активности
Solar activity is expected to be
generally low. There continues to be, however, a slight chance for
an isolated M-class flare.
IIA. Обзор геофизической активности от 29 - 2100Z до 30 - 2100Z
The geomagnetic field was initially quiet. An increase to unsettled
to active levels with some minor storm periods at high latitudes
occurred after 1003Z after a disturbance in the solar wind impacted
the magnetosphere. The disturbance was also seen at the ACE
spacecraft at about 0855Z: solar wind increased from around 280 km/s
to about 320 km/s, Bt from 3 nT up to about 6 nT, and density from
less than 1 p/cc up to about 6 p/cc. The solar wind parameters
continued to show somewhat elevated signatures for the remainder of
the period. There was also a solar sector boundary crossing on 29
October at about 2111Z from negative to positive polarity and the
presence of a positive sector was clearly indicated throughout the
interval. In addition, solar wind speed and temperature were showing
an increasing trend near the end of the interval. It appears that
the initial phase of the disturbance was related to the DSF/CME that
occurred on 26 October. However, it also appears that the expected
high speed stream is beginning to be evident in the solar wind
observations.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to be unsettled for the next 24 hours (31 October) with a
chance for active periods as the high speed stream is expected to be
more clearly evident. Quiet to unsettled levels are expected for the
second day (01 November) and quiet levels are expected to
predominate on the third day (02 November).
III. Вероятность события от 31 - Oct до 02 - Nov
M-класс | 10% | 10% | 10% |
X-класс | 01% | 01% | 01% |
Протон | 01% | 01% | 01% |
PCAF | Green
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 30 Oct 127
Прогнозируемый 31 Oct-02 Nov 130/130/125
среднее значение за последние 3 месяца 30 Oct 124
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 29 Oct 002/002
По оценкам Afr/Ap 30 Oct 007/008
Прогнозируемый Afr/Ap 31 Oct-02 Nov 010/010-005/008-005/005
VI. Вероятность геомагнитной активности с 31 - Oct до 02 - Nov
A. Средние широты |
Активно | 35% | 10% | 10% |
Слабый шторм | 10% | 05% | 05% |
Большой шторм | 05% | 01% | 01% |
B. Высокие широты |
Активно | 40% | 20% | 10% |
Слабый шторм | 25% | 15% | 05% |
Большой шторм | 15% | 05% | 01% |
Все время в UTC
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